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• W2290164171 abstract "Context. Until 2006, helium emission lines had never been observed in RR Lyrae stars. For the first time, a pre-maximum helium emission in 11 RRab stars was observed during rising light (around the pulsation phase 0.92) and the reappearance of helium emission near maximum light (phase 0.0) in one RRab star: RV Oct. This post-maximum emission has been only observed in the He I λ5875.66 (D3) line. Its intensity is very weak, and its profile mimics a P-Cygni profile with the emission peak centered at the laboratory wavelength. The physical explanation for this unexpected line profile has not been proposed yet." @default.
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• W2290164171 date "2016-03-01" @default.
• W2290164171 modified "2023-09-30" @default.
• W2290164171 title "A helium P-Cygni profile in RR Lyrae stars?" @default.
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• W2290164171 doi "https://doi.org/10.1051/0004-6361/201527287" @default.
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